Résumé / Abstract Seminaire_IAP
« Gravitational radiation from compact binary star systems »

Luc Blanchet

To be observed and analyzed by the gravitational wave detectors LIGO and VIRGO on ground and LISA in space, inspiralling compact binaries (binary star systems composed of neutron stars and/or black holes) require high-accuracy templates predicted by general relativity. These very relativistic systems are ideally suited for application of a high-order post-Newtonian gravitational wave generation formalism. In this talk, after general introduction and motivation, we shall review the current state of the art on post-Newtonian methods as applied to the motion and gravitational radiation of compact binary systems. We shall then present some recent work on the comparison between the post-Newtonian approximation and black hole perturbation theory as applied to compact binary systems with very small mass ratio. Finally we shall review the recent post-Newtonian calculations of the gravitational recoil of the black hole formed by coalescence of compact binary systems.
vendredi 16 septembre 2011 - 11:00
Salle des séminaires Évry Schatzman, Institut d'Astrophysique de Paris
Page web du séminaire / Seminar's webpage